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arxiv: astro-ph/9703191 · v1 · pith:IQNDB54Hnew · submitted 1997-03-28 · 🌌 astro-ph

LonGSp: the Gornergrat Longslit Infrared Spectrometer

classification 🌌 astro-ph
keywords spectrometeralongarcseccooledgornergratgratinginfraredlongsp
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We present a near-infrared cooled grating spectrometer that has been developed at the Arcetri Astrophysical Observatory for the 1.5 m Infrared Telescope at Gornergrat (TIRGO). The spectrometer is equipped with cooled reflective optics and a grating in Littrow configuration. The detector is an engineering grade Rockwell NICMOS3 array (256x256 pixels of 40 $\mu$m). The scale on the focal plane is 1.73 arcsec/pixel and the field of view along the slit is 70 arcsec. The accessible spectral range is 0.95-2.5 $\mu$m with a dispersion, at first order, of about 11.5 angstroms/pixel. This paper presents a complete description of the instrument, including its optics and cryo-mechanical system, along with astronomical results from test observations, started in 1994. Since January 1996, LonGSp is offered to TIRGO users and employed in several Galactic and extragalactic programs.

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